Abstract
Babul & Rees (1992; MNRAS, 255, 346, hereafter BR92) proposed an idea that low-mass galaxies experiencing their initial starburst at z 1 evolve into the present dwarf ellipticals and that the epoch of decline in the UV background determines when the initial starburst begins.
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© 1999 Springer Science+Business Media Dordrecht
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Atuko, N., Isibasi, N. (1999). Formation of Dwarf Galaxies by Delayed Star Formation. In: Miyama, S.M., Tomisaka, K., Hanawa, T. (eds) Numerical Astrophysics. Astrophysics and Space Science Library, vol 240. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-4780-4_23
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DOI: https://doi.org/10.1007/978-94-011-4780-4_23
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